J/ApJS/183/1     Catalog of central stellar velocity dispersions     (Ho+, 2009)

A search for "dwarf" Seyfert nuclei. VII. A catalog of central stellar velocity dispersions of nearby galaxies. Ho L.C., Greene J.E., Filippenko A.V., Sargent W.L.W. <Astrophys. J. Suppl. Ser., 183, 1-16 (2009)> =2009ApJS..183....1H 2009ApJS..183....1H
ADC_Keywords: Active gal. nuclei ; Velocity dispersion ; Spectroscopy ; Surveys Keywords: galaxies: active - galaxies: kinematics and dynamics - galaxies: nuclei - galaxies: Seyfert - galaxies: starburst - surveys Abstract: We present new central stellar velocity dispersion measurements for 428 galaxies in the Palomar spectroscopic survey of bright, northern galaxies. Of these, 142 have no previously published measurements, most being relatively late-type systems with low velocity dispersions (≲100km/s). We provide updates to a number of literature dispersions with large uncertainties. Our measurements are based on a direct pixel-fitting technique that can accommodate composite stellar populations by calculating an optimal linear combination of input stellar templates. The original Palomar survey data were taken under conditions that are not ideally suited for deriving stellar velocity dispersions for galaxies with a wide range of Hubble types. We describe an effective strategy to circumvent this complication and demonstrate that we can still obtain reliable velocity dispersions for this sample of well-studied nearby galaxies. Description: A full description of the Palomar survey is given by Ho et al. (1995, Cat. J/ApJS/98/477, 1997, Cat. J/ApJS/112/315). This survey covers a nearly complete, magnitude-limited sample of 486 galaxies from the Revised Shapley-Ames Catalog (Sandage & Tammann, 1981rsac.book.....S 1981rsac.book.....S, Cat. VII/51) that satisfies BT≤12.5mag and δ>0°. The spectra were acquired using the Double Spectrograph mounted at the Cassegrain focus of the Hale 5m telescope at Palomar Observatory. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 78 486 Catalog of stellar velocity dispersions -------------------------------------------------------------------------------- See also: VII/51 : Revised Shapley-Ames Catalog of Bright Galaxies (Sandage+, 1981) VII/72 : Catalog of Stellar Velocity Dispersions (Whitmore+ 1985) VII/237 : HYPERLEDA. I. Catalog of galaxies (Paturel+, 2003) J/ApJS/100/105 : Stellar velocity dispersions. II. (McElroy 1995) J/ApJS/98/477 : Optical spectral atlas of Seyfert nuclei (Ho+ 1995) J/ApJS/112/315 : Spectroscopic parameters of Seyfert nuclei (Ho+ 1997) J/A+AS/133/317 : Stellar kinematics in spiral galaxies (Heraudeau+ 1998) J/AJ/126/2268 : Velocity dispersions and Mg2 index of galaxies (Wegner+, 2003) J/A+A/408/873 : Gas and stellar kinematics in spirals (Corsini+, 2003) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Name Galaxy name 11- 15 F5.1 km/s sigL ? Literature velocity dispersion 17- 20 F4.1 km/s e_sigL ? Uncertainty in sigmaLit 22- 23 I2 --- r_sigL ? Reference on sigmaLit (1) 25- 29 F5.1 km/s sigB ? Palomar blue velocity dispersion 31- 34 F4.1 km/s e_sigB ? Uncertainty in sigmaPalB 36- 40 F5.1 km/s sigR ? Palomar red velocity dispersion 42- 45 F4.1 km/s e_sigR ? Uncertainty in sigmaPalR 47- 51 F5.1 km/s sigP ? Palomar final velocity dispersion 53- 56 F4.1 km/s e_sigP ? Uncertainty in sigmaPalF 58- 66 A9 --- Notes Additional notes on the Palomar dispersions (2) 68 A1 --- l_sig Limit flag on sigma 69- 73 F5.1 km/s sig ? Adopted velocity dispersion 75- 78 F4.1 km/s e_sig ? Uncertainty in sigma -------------------------------------------------------------------------------- Note (1): References as follows: 1 = Hyperleda (Cat. VII/237); 2 = Barth et al. (2002AJ....124.2607B 2002AJ....124.2607B); 3 = Kormendy & McClure (1993AJ....105.1793K 1993AJ....105.1793K); 4 = Ganda et al. (2006MNRAS.367...46G 2006MNRAS.367...46G); 5 = Wegner et al. (2003, Cat. J/AJ/126/2268); 6 = Batcheldor et al. (2005ApJS..160...76B 2005ApJS..160...76B); 7 = Heraudeau & Simien (1998, Cat. J/A+AS/133/317); 8 = Nelson et al. (2004ApJ...615..652N 2004ApJ...615..652N); 9 = Funes et al. (2002A&A...388...50F 2002A&A...388...50F); 10 = Sarzi et al. (2002ApJ...567..237S 2002ApJ...567..237S); 11 = Marconi et al. (2003ApJ...586..868M 2003ApJ...586..868M); 12 = Corsini et al. (2003, Cat. J/A+A/408/873); 13 = Filippenko & Ho (2003ApJ...588L..13F 2003ApJ...588L..13F). Note (2): Notes as follows: 1 = The adopted velocity dispersion was estimated from the [NII]6583Å emission line following the procedure of Ho (2009ApJ...699..638H 2009ApJ...699..638H). 2 = Stellar features too weak in the blue or red. 3 = Spectrum partly corrupted. 4 = The HyperLeda value of σ=240km/s pertains to the "southeast-northwest" component of this merging galaxy; the correct dispersion for the primary nucleus is σ=100±25km/s (see Section 3.4). 5 = Blue spectrum not available. 6 = Blue spectrum not well resolved. 7 = Red spectrum not well resolved. 8 = Blue fit unreliable. 9 = Red fit unreliable. 10 = G band corrupted in blue; masked out. 11 = The literature value corresponds to the central nuclear star cluster; the Palomar value is more representative of the central 2"x4" region. 12 = Velocity dispersion possibly overestimated slightly. -------------------------------------------------------------------------------- History: From electronic version of the journal References: Filippenko A.V. Paper I. 1985ApJS...57..503F 1985ApJS...57..503F Ho L.C. Paper II. 1995ApJS...98..477H 1995ApJS...98..477H Ho L.C. Paper III. 1997ApJS..112..315H 1997ApJS..112..315H. Cat. J/ApJS/112/315 Ho L.C. Paper IV. 1997ApJS..112..391H 1997ApJS..112..391H Ho L.C. Paper V. 1997ApJ...487..568H 1997ApJ...487..568H Ho L.C. Paper VI. 2003ApJ...583..159H 2003ApJ...583..159H
(End) Greg Schwarz [AAS], Emmanuelle Perret [CDS] 05-Jan-2010
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line